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53 Camelopardalis : ウィキペディア英語版 | 53 Camelopardalis
53 Camelopardalis is a spectroscopic binary in the constellation Camelopardalis. It is approximately 321 light years from Earth. The binary has an orbital period of 6.52 years. The primary component, 53 Camelopardalis A, is a white A-type main sequence dwarf with a mean apparent magnitude of +6.02. It is classified as an Alpha2 Canum Venaticorum type variable star and its brightness varies from magnitude +5.95 to +6.08 with a period of 8.03 days.
抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「53 Camelopardalis」の詳細全文を読む
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